Planned stereo pairs have suitable stereo convergence angles and illumination by design.
In addition to planned stereo pairs, the Pairendipity software can identify overlapping
HiRISE images that are serendipitously suitable for stereo processing and find stereo
pairs within the CTX dataset.
Planned HiRISE stereo pairs are listed in the “Stereo Pair List (CSV)” link below.
Since this list is based on produced stereo anaglyphs it also contains a few serendipitous
pairs that underwent special processing. Most serendipitous HiRISE stereo pairs are listed
in the “Pairendipity Stereo” link, while CTX stereo pairs are listed
in “Pairendipity CTX Stereo”.
Images taken close together in time minimize illumination and frost differences and are
especially useful (see the Delta-Days column in the Pairendipity files or difference
the orbit numbers in the image IDs in the Stereo Pair List file). Stereo pairs
with both images planned within the same 14-day (168-orbit) operations cycle are known as SPORCs.
| Aeolis Planum: ESP_023785_1745 ESP_067671_1745 (Interval in Earth days: 3420) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.55 | 154. | 0 | -21.5 | 32.9 | 41.2 |
| Rugged Banded Material in Crater in Northwest Hellas Planitia: ESP_023789_1420 ESP_024066_1420 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.7 | 47.4 | 21.8 | 0.082 | 44.7 | 50.6 |
| Gullies with Varied Shapes on a Crater Wall: ESP_023665_1410 ESP_024087_1410 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.5 | 194. | 6.50 | -2.95 | 44.2 | 51.6 |
| Libya Montes Layered Cliffs: ESP_023827_1835 ESP_024671_1835 (Interval in Earth days: 65) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.427 | 85.9 | 11.0 | -9.63 | 32.7 | 38.9 |
| South Polar Residual Cap in Late Summer: ESP_023677_0920 ESP_023781_0920 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.0 | 298. | 11.1 | 22.62 | 84.1 | 84.5 |
| Thumbprint Terrian in South Polar Residual Cap: ESP_023767_0925 ESP_023676_0925 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.3 | 323. | 16.8 | 3.381 | 84.0 | 84.1 |
| Ice-Rich Fill Deposits on Cerulli Crater Ejecta: ESP_023526_2135 ESP_023816_2135 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.17 | 21.5 | -6.2 | 16.62 | 51.2 | 46.4 |
| Impact Crater with Active Slope Processes: ESP_023809_1415 ESP_024099_1415 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.1 | 223. | -3.0 | 25.53 | 46.8 | 49.8 |
| Active Dune Gullies: ESP_023600_1095 ESP_024035_1095 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -70.3 | 178. | -3.9 | 13.86 | 67.7 | 74.4 |
| Well-Preserved Unnamed 6-Kilometer Diameter Crater in Daedalia Planum: ESP_023756_1600 ESP_051052_1600 (Interval in Earth days: 2127) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.9 | 227. | 5.42 | -8.70 | 35.6 | 47.0 |
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